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<ri:Resource created="2022-11-09T07:26:10Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Distance catalogue for AGB stars</title><shortName>J/A+A/667/A74</shortName><identifier>ivo://CDS.VizieR/J/A+A/667/A74</identifier><altIdentifier>doi:10.26093/cds/vizier.36670074</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Andriantsaralaza M.</name></creator><creator><name>Ramstedt S.</name></creator><creator><name>Vlemmings W.H.T</name></creator><creator><name>De Beck E.</name></creator><date role="Updated">2022-11-28T12:07:48Z</date><date role="Created">2022-11-09T07:26:10Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>variable-stars</subject><subject>giant-stars</subject><subject>stellar-distance</subject><subject>visible-astronomy</subject><description>Estimating the distances to asymptotic giant branch (AGB) stars using optical measurements of their parallaxes is not straightforward because of the large uncertainties introduced by their dusty envelopes, their large angular sizes, and their surface brightness variability. We compared the parallaxes from Gaia DR3 with parallaxes measured with maser observations with very long baseline interferometry (VLBI) to determine a statistical correction factor for the DR3 parallaxes using a sub-sample of 33 maser-emitting oxygen-rich nearby AGB stars. We then calculated the distances of a total of about 200 AGB stars in the DEATHSTAR project using a Bayesian statistical approach on the corrected DR3 parallaxes and a prior based on the previously determined Galactic distribution of AGB stars. We found that the derived Gaia distances are associated with significant, asymmetrical errors for more than 40% of the sources in our sample, and thus are unreliable for these sources. We performed radiative transfer modelling of the stellar and dust emission to determine the luminosity of the sources in the VLBI sub-sample based on the distances derived from maser parallaxes, and derived a new bolometric period-luminosity relation for Galactic oxygen-rich Mira variables. A new distance catalogue based on these results is provided for the sources in the DEATHSTAR sample.</description><source format="bibcode">2022A&amp;A...667A..74A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/667/A74</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/640/A133">J/A+A/640/A133 : DEATHSTAR. Nearby AGB stars with ALMA ACA (Ramstedt+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/653/A53">J/A+A/653/A53 : DEATHSTAR. II. 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